st clumps in the infrared dust bubble [CWP2007] CS 51. Use of Spitzer GLIMPSE and MIPSGAL data to identify N=93 YSOs towards the bubble. Use of archival 2MASS, Herschel and MALT90 survey data. | |
in source: | [CWP2007] CS 51 |
Ref: | =2017MNRAS.472.4750D |
by | DAS S.R. , TEJ A., VIG S., LIU H.-L., LIU T., ISHWARA CHANDRA C.H., GHOSH S.K. |
Mon. Not. R. Astron. Soc., 472, 4750-4768 (2017) | |
Infrared dust bubble CS51 and its interaction with the surrounding interstellar medium. | |
o | Fig. 4, Table 5: <[DTV2017] Star N> (Nos 1-5). Fig. 5, Table 6: <[DTV2017] Clump N> (Nos 1-5). Table A1: <[DTV2017] YSO NN> (Nos 1-93). |
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